Low Noise Non TE-Cooled Backthinned Spectrometer
• Scientific-grade high performance with low cost • Low dark noise and stray light • Good dynamic range and high signal to noise ratio • High Ultra-Violet Quantum Efficiency • Flexible optical input direct to slit or via fiber • Designed from the ground up for a wide range of applications • High speed data acquisition • Standard design allows up to 200-1050 nm range • Auto shutter for dark condition
FEATURE | VALUE |
---|---|
Detectors | Hamamatsu S10420-1106(Non TE-Cooled Backthinned FFT CCD) ▶ Number of Pixels : 2048 X 64 ▶ Sensing Pixel Size : 14 μm X 14 μm ▶ Well depth : 200Ke- ▶ Quantum efficiency : >90% @650 nm, 65% @250 nm |
Spectrograph # | 3.3 |
Dark Noise RMS | < 7 RMS counts @ 35 msec |
Signal to Noise Ratio | 450 : 1 |
Fiber Coupler | SMA905 of FC standard |
Wavelength Range | Full Range : 200 ~ 1050 nm UV Range : 200 ~ 450 nm VIS Range : 380 ~ 760 nm NIR Range : 550 ~ 1050 nm |
Order Sorting Filter | Longpass filter or linear variable filter installed per wavelength coverage |
Optical Resolution | 0.25 ~ 7 nm FWHM |
Stray Light Level | < 0.01% @632 nm (< 0.5% AVG) |
Computer Interface | USB 1.1/2.0 compatible |
Min. Exposure Time | 7 msec |
Trigger Mode | Free Run S/W Trigger H/W Trigger |
Operationg System | Windows 7/10 (32/64 bit) |
SDK Support | Visual C++ / Visual Basic / LabVIEW |
Dimensions / Weight | 152 mm X 100 mm X 63.6 mm / 1.2 Kg |
The Choice for Low Signal Level Applications
Korea Spectral Products is offering the new SM642 non TE cooled back-thinned 2048 pixel array CCD spectrometer.
The SM642 provides high quantum efficiency in UV and high dynamic range. The detector used in the SM642 has 2048 pixels and helps to get butter resolution. It is ideal for UV/ViS/NIR spectrometry that requires high signal to noise ratio and/or high dynamic range. The back-thinned CCD has excellent sensitivity in UV and allows deep UV application, even below 200nm. Well designed housing allows a wide measurement window like from 200nm to 1050nm (smaller measurement window sizes increase spectral resolution and light sensitivity) with low stray light.
Standard interface to the SM642 is a USB 1.1/2.0 compatible interface with 16-bit. Software support includes a SDK and DLLs for dedicated applications development and our SM32Pro Windows-based spectral acquisition and analysis software.
The new upgraded SM642 provides the auto-shutter function to make dark conditions automatically. Users don't need to block any input light for setting 0% transmission (dark scan).
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